50 citations · 120 across the 6 of their papers we have counts for
6 papers
Inner edges of planetesimal belts: collisionally eroded or truncated?
Amaia Imaz Blanco, Sebastian Marino, Luca Matrà +9
The radial structure of debris discs can encode important information about their dynamical and collisional history. In this paper we present a 3-phase analytical model to analyse…
The clumpy structure of Eridani's debris disc revisited by ALMA
Mark Booth, Tim D. Pearce, Alexander V. Krivov +8
Eridani is the closest star to our Sun known to host a debris disc. Prior observations in the (sub-)millimetre regime have potentially detected clumpy structure in the disc and…
Determining the Shape, Size, and Sources of the Zodiacal Dust Cloud using Polarized Ultraviolet Scattered Sunlight
Geoffrey Bryden, Neal J. Turner, Petr Pokorny +7
The solar system's Zodiacal Cloud is visible to the unaided eye, yet the origin of its constituent dust particles is not well understood, with a wide range of proposed divisions be…
Inner mean-motion resonances with eccentric planets: A possible origin for exozodiacal dust clouds
Virginie Faramaz, Steve Ertel, Mark Booth +2
High levels of dust have been detected in the immediate vicinity of many stars, both young and old. A promising scenario to explain the presence of this short-lived dust is that th…
94 Ceti: a triple star with a planet and dust disc
J. Wiegert, V. Faramaz, F. Cruz-Saenz de Miera
94 Ceti is a triple star system with a circumprimary gas giant planet and far-infrared excess. Such excesses around main sequence stars are likely due to debris discs, and are cons…
Insights on the dynamical history of the Fomalhaut system - Investigating the Fom c hypothesis
Virginie Faramaz, Hervé Beust, Jean-Charles Augereau +2
The eccentric shape of the debris disk observed around Fomalhaut was first attributed to Fom b, a companion detected near the belt inner-edge, but new constraints on its orbit reve…